Quintessential inflation and cosmological seesaw mechanism: reheating and observational constraints
Cita com:
hdl:2117/352892
Document typeArticle
Defense date2021-07
Rights accessOpen Access
Except where otherwise noted, content on this work
is licensed under a Creative Commons license
:
Attribution-NonCommercial-NoDerivs 3.0 Spain
Abstract
Recently a new kind of quintessential inflation coming from the Lorentzian distribution has been introduced in [1,2]. The model leads to a very simple potential, which basically depends on two parameters, belonging to the class of a-attractors and depicting correctly the early and late time accelerations of our universe. The potential emphasizes a cosmological seesaw mechanism (CSSM) that produces a large inflationary vacuum energy in one side of the potential and a very small value of dark energy on the right hand side of the potential. Here we show that the model agrees with the recent observations and with the reheating constraints. Therefore the model gives a reasonable scenario beyond the standard ¿CDM that includes the inflationary epoch
CitationAresté, L. [et al.]. Quintessential inflation and cosmological seesaw mechanism: reheating and observational constraints. "Journal of cosmology and astroparticle physics", Juliol 2021, vol. 2021, núm. 7.
ISSN1475-7516
Publisher versionhttps://iopscience.iop.org/article/10.1088/1475-7516/2021/07/007
Other identifiershttps://arxiv.org/abs/2102.09514v2
Files | Description | Size | Format | View |
---|---|---|---|---|
Cosmological Seesaw Mechanism.pdf | 955,3Kb | View/Open |